Qing Du , Jiyuan Yin , Wenjiao Xiao , Tao Wang , Mike Fowler , Zhiyong Zhu , Zaili Tao , Guibin Zhang , Min Sun , Guochun Zhao
{"title":"稀土伟晶岩成因的地球化学、热力学和Li同位素约束:地壳Li循环的意义","authors":"Qing Du , Jiyuan Yin , Wenjiao Xiao , Tao Wang , Mike Fowler , Zhiyong Zhu , Zaili Tao , Guibin Zhang , Min Sun , Guochun Zhao","doi":"10.1016/j.gloplacha.2025.105029","DOIUrl":null,"url":null,"abstract":"<div><div>Rare-metal pegmatite deposits are widespread in collisional settings around the world and are increasingly important to the global requirement for critical metals. However, their genesis and rare-metal enrichment processes remain enigmatic, particularly concerning whether they originate from highly fractionated granitic magmas or anatexis of metasedimentary rocks. In this study, we integrate zircon U<img>Pb geochronology, whole-rock and mineral chemistry and Li isotopic compositions of pegmatites and associated granitoids from the West Kunlun Orogenic Belt (WKOB) in northern Tibetan Plateau, to investigate these issues. Zircon U<img>Pb dating yields weighted mean ages of 223 Ma for the pegmatites and 213–222 Ma for the adjacent granitoids. Compared with the granitoids, the pegmatites exhibit distinct geochemical signatures, including high SiO<sub>2</sub> (72.9–74.5 wt%) and Al<sub>2</sub>O<sub>3</sub> (16.2–17.2 wt%), low TiO<sub>2</sub> (<0.01 wt%), <sup>T</sup>Fe<sub>2</sub>O<sub>3</sub> (0.09–0.21 wt%) and MgO (<0.02 wt%), and strongly peraluminous signatures (A/CNK = 1.04–2.56). δ<sup>7</sup>Li values of Li-rich pegmatites and Li-poor pegmatites are relatively uniform (+2.11 to +0.8 ‰), but for muscovite the δ<sup>7</sup>Li values extend to lower values in Li-poor than Li-rich pegmatites (−2.93 to +2.11 ‰ and + 0.37 to +2.98 ‰, respectively). The absence of coherent fractionation trends between pegmatites and granitoids (e.g., Rb, Cs), along with a lack of mineralogical evidence for extreme magmatic differentiation, argues against a fractionated granite origin. Instead, Li isotope models of partial melting, thermodynamically-defined phase equilibria and associated elemental calculations all demonstrate that the West Kunlun Li-rich pegmatites were likely generated by melting of Li-rich claystone under amphibolite facies conditions, whereas the Li-poor pegmatites originated from typical metasedimentary sources. We propose that the involvement of Li-rich claystone into the middle to lower crust during collisional orogenesis was a key control on the formation of Li-rich pegmatites in the WKOB. This mechanism highlights the metallogenic significance of crustal-scale Li cycling and may be broadly applicable to rare metal pegmatite systems in other collisional orogenic belts.</div></div>","PeriodicalId":55089,"journal":{"name":"Global and Planetary Change","volume":"254 ","pages":"Article 105029"},"PeriodicalIF":4.0000,"publicationDate":"2025-08-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Geochemical, thermodynamic and Li isotope constraints on the genesis of rare-metal pegmatites: Implications for crustal Li cycling\",\"authors\":\"Qing Du , Jiyuan Yin , Wenjiao Xiao , Tao Wang , Mike Fowler , Zhiyong Zhu , Zaili Tao , Guibin Zhang , Min Sun , Guochun Zhao\",\"doi\":\"10.1016/j.gloplacha.2025.105029\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>Rare-metal pegmatite deposits are widespread in collisional settings around the world and are increasingly important to the global requirement for critical metals. However, their genesis and rare-metal enrichment processes remain enigmatic, particularly concerning whether they originate from highly fractionated granitic magmas or anatexis of metasedimentary rocks. In this study, we integrate zircon U<img>Pb geochronology, whole-rock and mineral chemistry and Li isotopic compositions of pegmatites and associated granitoids from the West Kunlun Orogenic Belt (WKOB) in northern Tibetan Plateau, to investigate these issues. Zircon U<img>Pb dating yields weighted mean ages of 223 Ma for the pegmatites and 213–222 Ma for the adjacent granitoids. Compared with the granitoids, the pegmatites exhibit distinct geochemical signatures, including high SiO<sub>2</sub> (72.9–74.5 wt%) and Al<sub>2</sub>O<sub>3</sub> (16.2–17.2 wt%), low TiO<sub>2</sub> (<0.01 wt%), <sup>T</sup>Fe<sub>2</sub>O<sub>3</sub> (0.09–0.21 wt%) and MgO (<0.02 wt%), and strongly peraluminous signatures (A/CNK = 1.04–2.56). δ<sup>7</sup>Li values of Li-rich pegmatites and Li-poor pegmatites are relatively uniform (+2.11 to +0.8 ‰), but for muscovite the δ<sup>7</sup>Li values extend to lower values in Li-poor than Li-rich pegmatites (−2.93 to +2.11 ‰ and + 0.37 to +2.98 ‰, respectively). The absence of coherent fractionation trends between pegmatites and granitoids (e.g., Rb, Cs), along with a lack of mineralogical evidence for extreme magmatic differentiation, argues against a fractionated granite origin. Instead, Li isotope models of partial melting, thermodynamically-defined phase equilibria and associated elemental calculations all demonstrate that the West Kunlun Li-rich pegmatites were likely generated by melting of Li-rich claystone under amphibolite facies conditions, whereas the Li-poor pegmatites originated from typical metasedimentary sources. We propose that the involvement of Li-rich claystone into the middle to lower crust during collisional orogenesis was a key control on the formation of Li-rich pegmatites in the WKOB. This mechanism highlights the metallogenic significance of crustal-scale Li cycling and may be broadly applicable to rare metal pegmatite systems in other collisional orogenic belts.</div></div>\",\"PeriodicalId\":55089,\"journal\":{\"name\":\"Global and Planetary Change\",\"volume\":\"254 \",\"pages\":\"Article 105029\"},\"PeriodicalIF\":4.0000,\"publicationDate\":\"2025-08-21\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Global and Planetary Change\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0921818125003388\",\"RegionNum\":1,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"GEOGRAPHY, PHYSICAL\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Global and Planetary Change","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0921818125003388","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOGRAPHY, PHYSICAL","Score":null,"Total":0}
Geochemical, thermodynamic and Li isotope constraints on the genesis of rare-metal pegmatites: Implications for crustal Li cycling
Rare-metal pegmatite deposits are widespread in collisional settings around the world and are increasingly important to the global requirement for critical metals. However, their genesis and rare-metal enrichment processes remain enigmatic, particularly concerning whether they originate from highly fractionated granitic magmas or anatexis of metasedimentary rocks. In this study, we integrate zircon UPb geochronology, whole-rock and mineral chemistry and Li isotopic compositions of pegmatites and associated granitoids from the West Kunlun Orogenic Belt (WKOB) in northern Tibetan Plateau, to investigate these issues. Zircon UPb dating yields weighted mean ages of 223 Ma for the pegmatites and 213–222 Ma for the adjacent granitoids. Compared with the granitoids, the pegmatites exhibit distinct geochemical signatures, including high SiO2 (72.9–74.5 wt%) and Al2O3 (16.2–17.2 wt%), low TiO2 (<0.01 wt%), TFe2O3 (0.09–0.21 wt%) and MgO (<0.02 wt%), and strongly peraluminous signatures (A/CNK = 1.04–2.56). δ7Li values of Li-rich pegmatites and Li-poor pegmatites are relatively uniform (+2.11 to +0.8 ‰), but for muscovite the δ7Li values extend to lower values in Li-poor than Li-rich pegmatites (−2.93 to +2.11 ‰ and + 0.37 to +2.98 ‰, respectively). The absence of coherent fractionation trends between pegmatites and granitoids (e.g., Rb, Cs), along with a lack of mineralogical evidence for extreme magmatic differentiation, argues against a fractionated granite origin. Instead, Li isotope models of partial melting, thermodynamically-defined phase equilibria and associated elemental calculations all demonstrate that the West Kunlun Li-rich pegmatites were likely generated by melting of Li-rich claystone under amphibolite facies conditions, whereas the Li-poor pegmatites originated from typical metasedimentary sources. We propose that the involvement of Li-rich claystone into the middle to lower crust during collisional orogenesis was a key control on the formation of Li-rich pegmatites in the WKOB. This mechanism highlights the metallogenic significance of crustal-scale Li cycling and may be broadly applicable to rare metal pegmatite systems in other collisional orogenic belts.
期刊介绍:
The objective of the journal Global and Planetary Change is to provide a multi-disciplinary overview of the processes taking place in the Earth System and involved in planetary change over time. The journal focuses on records of the past and current state of the earth system, and future scenarios , and their link to global environmental change. Regional or process-oriented studies are welcome if they discuss global implications. Topics include, but are not limited to, changes in the dynamics and composition of the atmosphere, oceans and cryosphere, as well as climate change, sea level variation, observations/modelling of Earth processes from deep to (near-)surface and their coupling, global ecology, biogeography and the resilience/thresholds in ecosystems.
Key criteria for the consideration of manuscripts are (a) the relevance for the global scientific community and/or (b) the wider implications for global scale problems, preferably combined with (c) having a significance beyond a single discipline. A clear focus on key processes associated with planetary scale change is strongly encouraged.
Manuscripts can be submitted as either research contributions or as a review article. Every effort should be made towards the presentation of research outcomes in an understandable way for a broad readership.